Table 5: $\eta$ Boo squared visibilities.
Julian Date Stations N B (m) Az. ( $\deg$ ) $V^2 \pm {\rm stat} \pm {\rm syst}$ Calibrators

2 452 760.684 B3-M0 131 134.046 64.22 $0.3167\pm0.0187\pm0.0119$ $\alpha$ Crt

2 452 760.696 B3-M0 50 136.318 63.31 $0.3227\pm0.0415\pm0.0121$ $\alpha$ Crt

2 452 763.693 B3-M0 187 137.132 62.88 $0.3095\pm0.0092\pm0.0064$ $\mu$ Vir

**Table 5:** $\eta$ Boo squared visibilities.
Julian Date	Stations	N	B (m)	Az. ( $\deg$ )	$V^2 \pm {\rm stat} \pm {\rm syst}$	Calibrators
2 452 760.684	B3-M0	131	134.046	64.22	$0.3167\pm0.0187\pm0.0119$	$\alpha$ Crt
2 452 760.696	B3-M0	50	136.318	63.31	$0.3227\pm0.0415\pm0.0121$	$\alpha$ Crt
2 452 763.693	B3-M0	187	137.132	62.88	$0.3095\pm0.0092\pm0.0064$	$\mu$ Vir

Source LaTeX | All tables | In the text

	1 Introduction
	2 Global characteristics of the stars
	3 Diameter interferometric measurements
	4 Models and results
	5 Concluding remarks
	References